SEARCH for TeV GAMMA-RAY EMISSION from POINT-LIKE SOURCES in the INNER GALACTIC PLANE with A PARTIAL CONFIGURATION of the HAWC OBSERVATORY

A. U. Abeysekara; R. Alfaro; C. Alvarez; J. D. Alvarez; R. Arceo; J. C. Arteaga-Velá Zquez; H. A.Ayala Solares; A. S. Barber; B. M. Baughman; N. Bautista-Elivar; A. D.Becerril Reyes; E. Belmont; S. Y. Benzvi; A. Bernal; J. Braun; K. S. Caballero-Mora; T. Capistrán; A. Carraminana; S. Casanova; M. Castillo; U. Cotti; J. Cotzomi; S. Coutińo De León; E. De La Fuente; C. De León; T. Deyoung; R. Diaz Hernandez; B. L. Dingus; M. A. Duvernois; R. W. Ellsworth; O. Enriquez-Rivera; D. W. Fiorino; N. Fraija; F. Garfias; M. M. González; J. A. Goodman; M. Gussert; Z. Hampel-Arias; J. P. Harding; S. Hernandez; P. Hüntemeyer; C. M. Hui; A. Imran; A. Iriarte; P. Karn; D. Kieda; A. Lara; R. J. Lauer; W. H. Lee; D. Lennarz; H. León Vargas; J. T. Linnemann; M. Longo; G. Luis Raya; K. Malone; A. Marinelli; S. S. Marinelli; H. Martinez; O. Martinez; J. Martinez-Castro; J. A. Matthews; P. Miranda-Romagnoli; E. Moreno; M. Mostafá; L. Nellen; M. Newbold; R. Noriega-Papaqui; B. Patricelli; R. Pelayo; E. G. Pérez-Pérez; J. Pretz; Z. Ren; C. Riviere; D. Rosa-González; H. Salazar; F. Salesa Greus; A. Sandoval; M. Schneider; G. Sinnis; A. J. Smith; K. Sparks Woodle; R. W. Springer; I. Taboada; O. Tibolla; K. Tollefson; I. Torres; T. N. Ukwatta; L. Villasenor; K. Vrabel; T. Weisgarber; S. Westerhoff; I. G. Wisher; J. Wood; T. Yapici; G. B. Yodh; P. W. Younk; D. Zaborov; A. Zepeda; H. Zhou

doi:10.3847/0004-637X/817/1/3

SEARCH for TeV GAMMA-RAY EMISSION from POINT-LIKE SOURCES in the INNER GALACTIC PLANE with A PARTIAL CONFIGURATION of the HAWC OBSERVATORY

A. U. Abeysekara, R. Alfaro, C. Alvarez, J. D. Alvarez, R. Arceo, J. C. Arteaga-Velá Zquez, H. A.Ayala Solares, A. S. Barber, B. M. Baughman, N. Bautista-Elivar, A. D.Becerril Reyes, E. Belmont, S. Y. Benzvi, A. Bernal, J. Braun, K. S. Caballero-Mora, T. Capistrán, A. Carraminana, S. Casanova, M. CastilloU. Cotti, J. Cotzomi, S. Coutińo De León, E. De La Fuente, C. De León, T. Deyoung, R. Diaz Hernandez, B. L. Dingus, M. A. Duvernois, R. W. Ellsworth, O. Enriquez-Rivera, D. W. Fiorino, N. Fraija, F. Garfias, M. M. González, J. A. Goodman, M. Gussert, Z. Hampel-Arias, J. P. Harding, S. Hernandez, P. Hüntemeyer, C. M. Hui, A. Imran, A. Iriarte, P. Karn, D. Kieda, A. Lara, R. J. Lauer, W. H. Lee, D. Lennarz, H. León Vargas, J. T. Linnemann, M. Longo, G. Luis Raya, K. Malone, A. Marinelli, S. S. Marinelli, H. Martinez, O. Martinez, J. Martinez-Castro, J. A. Matthews, P. Miranda-Romagnoli, E. Moreno, M. Mostafá, L. Nellen, M. Newbold, R. Noriega-Papaqui, B. Patricelli, R. Pelayo, E. G. Pérez-Pérez, J. Pretz, Z. Ren, C. Riviere, D. Rosa-González, H. Salazar, F. Salesa Greus, A. Sandoval, M. Schneider, G. Sinnis, A. J. Smith, K. Sparks Woodle, R. W. Springer, I. Taboada, O. Tibolla, K. Tollefson, I. Torres, T. N. Ukwatta, L. Villasenor, K. Vrabel, T. Weisgarber, S. Westerhoff, I. G. Wisher, J. Wood, T. Yapici, G. B. Yodh, P. W. Younk, D. Zaborov, A. Zepeda, H. Zhou

Producción científica: Contribución a una revista › Artículo de revisión › revisión exhaustiva

34 Citas (Scopus)

Resumen

A survey of the inner Galaxy region of Galactic longitude l ∈[+15,+50] and latitude b ∈ [-4, +4] is performed using one-third of the High Altitude Water Cherenkov Observatory, operated during ts construction phase. To address the ambiguities arising from unresolved sources in the data, we use a maximum likelihood technique to identify point source candidates. Ten sources and candidate sources are identified in this analysis. Eight of these are associated with known TeV sources but not all have ifferential fluxes that are compatible with previous measurements. Three sources are detected with significances >5 sigma; after accounting for statistical trials, and are associated with known TeV sources.

Idioma original	Inglés
Número de artículo	3
Publicación	Astrophysical Journal
Volumen	817
N.º	1
DOI	https://doi.org/10.3847/0004-637X/817/1/3
Estado	Publicada - 20 ene. 2016

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Abeysekara, A. U., Alfaro, R., Alvarez, C., Alvarez, J. D., Arceo, R., Arteaga-Velá Zquez, J. C., Solares, H. A. A., Barber, A. S., Baughman, B. M., Bautista-Elivar, N., Reyes, A. D. B., Belmont, E., Benzvi, S. Y., Bernal, A., Braun, J., Caballero-Mora, K. S., Capistrán, T., Carraminana, A., Casanova, S., ... Zhou, H. (2016). SEARCH for TeV GAMMA-RAY EMISSION from POINT-LIKE SOURCES in the INNER GALACTIC PLANE with A PARTIAL CONFIGURATION of the HAWC OBSERVATORY. Astrophysical Journal, 817(1), Artículo 3. https://doi.org/10.3847/0004-637X/817/1/3

@article{ab962ee1a46f4862ac215f0e57449fcf,

title = "SEARCH for TeV GAMMA-RAY EMISSION from POINT-LIKE SOURCES in the INNER GALACTIC PLANE with A PARTIAL CONFIGURATION of the HAWC OBSERVATORY",

abstract = "A survey of the inner Galaxy region of Galactic longitude l ∈[+15,+50] and latitude b ∈ [-4, +4] is performed using one-third of the High Altitude Water Cherenkov Observatory, operated during ts construction phase. To address the ambiguities arising from unresolved sources in the data, we use a maximum likelihood technique to identify point source candidates. Ten sources and candidate sources are identified in this analysis. Eight of these are associated with known TeV sources but not all have ifferential fluxes that are compatible with previous measurements. Three sources are detected with significances >5 sigma; after accounting for statistical trials, and are associated with known TeV sources.",

keywords = "astroparticle physics, gamma rays: diffuse background, gamma rays: general",

author = "Abeysekara, {A. U.} and R. Alfaro and C. Alvarez and Alvarez, {J. D.} and R. Arceo and {Arteaga-Vel{\'a} Zquez}, {J. C.} and Solares, {H. A.Ayala} and Barber, {A. S.} and Baughman, {B. M.} and N. Bautista-Elivar and Reyes, {A. D.Becerril} and E. Belmont and Benzvi, {S. Y.} and A. Bernal and J. Braun and Caballero-Mora, {K. S.} and T. Capistr{\'a}n and A. Carraminana and S. Casanova and M. Castillo and U. Cotti and J. Cotzomi and Le{\'o}n, {S. Couti{\'n}o De} and Fuente, {E. De La} and Le{\'o}n, {C. De} and T. Deyoung and {Diaz Hernandez}, R. and Dingus, {B. L.} and Duvernois, {M. A.} and Ellsworth, {R. W.} and O. Enriquez-Rivera and Fiorino, {D. W.} and N. Fraija and F. Garfias and Gonz{\'a}lez, {M. M.} and Goodman, {J. A.} and M. Gussert and Z. Hampel-Arias and Harding, {J. P.} and S. Hernandez and P. H{\"u}ntemeyer and Hui, {C. M.} and A. Imran and A. Iriarte and P. Karn and D. Kieda and A. Lara and Lauer, {R. J.} and Lee, {W. H.} and D. Lennarz and Vargas, {H. Le{\'o}n} and Linnemann, {J. T.} and M. Longo and Raya, {G. Luis} and K. Malone and A. Marinelli and Marinelli, {S. S.} and H. Martinez and O. Martinez and J. Martinez-Castro and Matthews, {J. A.} and P. Miranda-Romagnoli and E. Moreno and M. Mostaf{\'a} and L. Nellen and M. Newbold and R. Noriega-Papaqui and B. Patricelli and R. Pelayo and P{\'e}rez-P{\'e}rez, {E. G.} and J. Pretz and Z. Ren and C. Riviere and D. Rosa-Gonz{\'a}lez and H. Salazar and Greus, {F. Salesa} and A. Sandoval and M. Schneider and G. Sinnis and Smith, {A. J.} and Woodle, {K. Sparks} and Springer, {R. W.} and I. Taboada and O. Tibolla and K. Tollefson and I. Torres and Ukwatta, {T. N.} and L. Villasenor and K. Vrabel and T. Weisgarber and S. Westerhoff and Wisher, {I. G.} and J. Wood and T. Yapici and Yodh, {G. B.} and Younk, {P. W.} and D. Zaborov and A. Zepeda and H. Zhou",

year = "2016",

month = jan,

day = "20",

doi = "10.3847/0004-637X/817/1/3",

language = "Ingl{\'e}s",

volume = "817",

journal = "Astrophysical Journal",

issn = "0004-637X",

number = "1",

}

Abeysekara, AU, Alfaro, R, Alvarez, C, Alvarez, JD, Arceo, R, Arteaga-Velá Zquez, JC, Solares, HAA, Barber, AS, Baughman, BM, Bautista-Elivar, N, Reyes, ADB, Belmont, E, Benzvi, SY, Bernal, A, Braun, J, Caballero-Mora, KS, Capistrán, T, Carraminana, A, Casanova, S, Castillo, M, Cotti, U, Cotzomi, J, León, SCD, Fuente, EDL, León, CD, Deyoung, T, Diaz Hernandez, R, Dingus, BL, Duvernois, MA, Ellsworth, RW, Enriquez-Rivera, O, Fiorino, DW, Fraija, N, Garfias, F, González, MM, Goodman, JA, Gussert, M, Hampel-Arias, Z, Harding, JP, Hernandez, S, Hüntemeyer, P, Hui, CM, Imran, A, Iriarte, A, Karn, P, Kieda, D, Lara, A, Lauer, RJ, Lee, WH, Lennarz, D, Vargas, HL, Linnemann, JT, Longo, M, Raya, GL, Malone, K, Marinelli, A, Marinelli, SS, Martinez, H, Martinez, O, Martinez-Castro, J, Matthews, JA, Miranda-Romagnoli, P, Moreno, E, Mostafá, M, Nellen, L, Newbold, M, Noriega-Papaqui, R, Patricelli, B, Pelayo, R, Pérez-Pérez, EG, Pretz, J, Ren, Z, Riviere, C, Rosa-González, D, Salazar, H, Greus, FS, Sandoval, A, Schneider, M, Sinnis, G, Smith, AJ, Woodle, KS, Springer, RW, Taboada, I, Tibolla, O, Tollefson, K, Torres, I, Ukwatta, TN, Villasenor, L, Vrabel, K, Weisgarber, T, Westerhoff, S, Wisher, IG, Wood, J, Yapici, T, Yodh, GB, Younk, PW, Zaborov, D, Zepeda, A & Zhou, H 2016, 'SEARCH for TeV GAMMA-RAY EMISSION from POINT-LIKE SOURCES in the INNER GALACTIC PLANE with A PARTIAL CONFIGURATION of the HAWC OBSERVATORY', Astrophysical Journal, vol. 817, n.º 1, 3. https://doi.org/10.3847/0004-637X/817/1/3

TY - JOUR

T1 - SEARCH for TeV GAMMA-RAY EMISSION from POINT-LIKE SOURCES in the INNER GALACTIC PLANE with A PARTIAL CONFIGURATION of the HAWC OBSERVATORY

AU - Abeysekara, A. U.

AU - Alfaro, R.

AU - Alvarez, C.

AU - Alvarez, J. D.

AU - Arceo, R.

AU - Arteaga-Velá Zquez, J. C.

AU - Solares, H. A.Ayala

AU - Barber, A. S.

AU - Baughman, B. M.

AU - Bautista-Elivar, N.

AU - Reyes, A. D.Becerril

AU - Belmont, E.

AU - Benzvi, S. Y.

AU - Bernal, A.

AU - Braun, J.

AU - Caballero-Mora, K. S.

AU - Capistrán, T.

AU - Carraminana, A.

AU - Casanova, S.

AU - Castillo, M.

AU - Cotti, U.

AU - Cotzomi, J.

AU - León, S. Coutińo De

AU - Fuente, E. De La

AU - León, C. De

AU - Deyoung, T.

AU - Diaz Hernandez, R.

AU - Dingus, B. L.

AU - Duvernois, M. A.

AU - Ellsworth, R. W.

AU - Enriquez-Rivera, O.

AU - Fiorino, D. W.

AU - Fraija, N.

AU - Garfias, F.

AU - González, M. M.

AU - Goodman, J. A.

AU - Gussert, M.

AU - Hampel-Arias, Z.

AU - Harding, J. P.

AU - Hernandez, S.

AU - Hüntemeyer, P.

AU - Hui, C. M.

AU - Imran, A.

AU - Iriarte, A.

AU - Karn, P.

AU - Kieda, D.

AU - Lara, A.

AU - Lauer, R. J.

AU - Lee, W. H.

AU - Lennarz, D.

AU - Vargas, H. León

AU - Linnemann, J. T.

AU - Longo, M.

AU - Raya, G. Luis

AU - Malone, K.

AU - Marinelli, A.

AU - Marinelli, S. S.

AU - Martinez, H.

AU - Martinez, O.

AU - Martinez-Castro, J.

AU - Matthews, J. A.

AU - Miranda-Romagnoli, P.

AU - Moreno, E.

AU - Mostafá, M.

AU - Nellen, L.

AU - Newbold, M.

AU - Noriega-Papaqui, R.

AU - Patricelli, B.

AU - Pelayo, R.

AU - Pérez-Pérez, E. G.

AU - Pretz, J.

AU - Ren, Z.

AU - Riviere, C.

AU - Rosa-González, D.

AU - Salazar, H.

AU - Greus, F. Salesa

AU - Sandoval, A.

AU - Schneider, M.

AU - Sinnis, G.

AU - Smith, A. J.

AU - Woodle, K. Sparks

AU - Springer, R. W.

AU - Taboada, I.

AU - Tibolla, O.

AU - Tollefson, K.

AU - Torres, I.

AU - Ukwatta, T. N.

AU - Villasenor, L.

AU - Vrabel, K.

AU - Weisgarber, T.

AU - Westerhoff, S.

AU - Wisher, I. G.

AU - Wood, J.

AU - Yapici, T.

AU - Yodh, G. B.

AU - Younk, P. W.

AU - Zaborov, D.

AU - Zepeda, A.

AU - Zhou, H.

PY - 2016/1/20

Y1 - 2016/1/20

N2 - A survey of the inner Galaxy region of Galactic longitude l ∈[+15,+50] and latitude b ∈ [-4, +4] is performed using one-third of the High Altitude Water Cherenkov Observatory, operated during ts construction phase. To address the ambiguities arising from unresolved sources in the data, we use a maximum likelihood technique to identify point source candidates. Ten sources and candidate sources are identified in this analysis. Eight of these are associated with known TeV sources but not all have ifferential fluxes that are compatible with previous measurements. Three sources are detected with significances >5 sigma; after accounting for statistical trials, and are associated with known TeV sources.

AB - A survey of the inner Galaxy region of Galactic longitude l ∈[+15,+50] and latitude b ∈ [-4, +4] is performed using one-third of the High Altitude Water Cherenkov Observatory, operated during ts construction phase. To address the ambiguities arising from unresolved sources in the data, we use a maximum likelihood technique to identify point source candidates. Ten sources and candidate sources are identified in this analysis. Eight of these are associated with known TeV sources but not all have ifferential fluxes that are compatible with previous measurements. Three sources are detected with significances >5 sigma; after accounting for statistical trials, and are associated with known TeV sources.

KW - astroparticle physics

KW - gamma rays: diffuse background

KW - gamma rays: general

UR - http://www.scopus.com/inward/record.url?scp=84955470282&partnerID=8YFLogxK

U2 - 10.3847/0004-637X/817/1/3

DO - 10.3847/0004-637X/817/1/3

M3 - Artículo de revisión

SN - 0004-637X

VL - 817

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 3

ER -

SEARCH for TeV GAMMA-RAY EMISSION from POINT-LIKE SOURCES in the INNER GALACTIC PLANE with A PARTIAL CONFIGURATION of the HAWC OBSERVATORY

Resumen

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